We present preliminary results on variable stars of a STARE's three month observational run centered at the Cygnus constellation. A total amount of aprox. 14000 stars with 9 < R < 12.5 magnitude, in STARE's 6.1 x 6.1.degrees(2) FOV, have been analyzed to obtain lightcurves for each of these stars. The data spans for similar to 90 nights. In this single field, we detect more that 40 stars with pulsation modes between 5 and 40 c/d, the vast mayority previously unknown to be variables.